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The Bargmann-Wigner Equation

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<strong>The</strong> <strong>Bargmann</strong>-<strong>Wigner</strong> <strong>Equation</strong>:<br />

Filed equation for arbitrary spin<br />

Farzad Qassemi<br />

IPM School and Workshop on Cosmology<br />

2-9 June, IPM, Tehran, Iran


Motivation<br />

◦ De-Broglie fusion theory of light:<br />

1) It was motivated by De Broglie to derive<br />

Maxwell’s equation as emergence field<br />

equation of two spin ½ massless<br />

particles (Neutrino in that time)<br />

2) <strong>Bargmann</strong> and <strong>Wigner</strong> in their seminal<br />

paper in 1948 group theoretically<br />

speaking, generalize this approach to<br />

the field equation for arbitrary spin


Review<br />

◦ Dirac equation:<br />

(γ.<br />

∂ + m)ψ =<br />

0<br />

◦ Set of Gamma matrices<br />

I<br />

, γ , γ , γ γ , σ<br />

5 µ 5 µ µν<br />

Note: they form a complete set.


Charge conjugation operator<br />

*<br />

Cψ =ψ<br />

C<br />

−1<br />

γ<br />

5 5<br />

Cγ =<br />

T<br />

C γ C<br />

−1<br />

= −γ<br />

µ µ


Procedure<br />

1) We symmetries spinor of rank “n” ,<br />

2) It satisfies Dirac equation for each<br />

spinor index:<br />

ψ αβ..<br />

( γ.<br />

∂ + m)<br />

ψ αα α ' β ...<br />

'<br />

=<br />

0


Spin-1 Particle<br />

◦ Group theoretically speaking, the<br />

symmetric state of two spin-½<br />

particles gives spin-1particle. B-W<br />

method helps us to derive the field<br />

equation corresponding to new field<br />

equation. In spin-1 case it means<br />

we can derive Maxwell’s (Proca)<br />

equation from Dirac equation!


Spin-1<br />

ψ<br />

µ<br />

µν<br />

αβ<br />

= A ( γ σ<br />

µ<br />

C)<br />

αβ<br />

+ F (<br />

µνC)<br />

αβ<br />

◦ Now we contract above equation with;<br />

( C<br />

γ ) ,( C γ ) ,( C )<br />

−1 −1<br />

−1<br />

5 βδ 5γ ν βδ<br />

βδ


Spin-3/2 (Rarita-Schwinger eq)<br />

◦ We can continue to make a spin 3/2<br />

particle as follow;<br />

ραβ<br />

µ<br />

ρ<br />

µ<br />

αβ<br />

µν<br />

ψ = A ( γ C)<br />

+ F ( σ C)<br />

ρ<br />

µν<br />

αβ<br />

◦ Follow the same method of contraction.


Modified BW<br />

◦ Q: We examine if fully antisymmetrization<br />

spinor gives us<br />

what we expect.<br />

◦ A: Yes.


Spin-0<br />

◦ Here we try to (re)derive Klein-<br />

Gordon equation from second rank<br />

anti-symmetric spinor.<br />

◦ <strong>The</strong> general method is as before,<br />

except we changed the expansion of<br />

the spinor with respect to antisymmetric<br />

gamma matrices.


Spin-0<br />

ψ = A + )<br />

αβ<br />

ν<br />

( γ<br />

5C)<br />

αβ<br />

+ B ( γ<br />

5γνC)<br />

αβ<br />

F(<br />

C<br />

αβ<br />

◦ Now, we contract above spinor with<br />

symmetric gamma matrices.<br />

( C<br />

−1 −1<br />

µ<br />

)<br />

βδ<br />

,( C σ<br />

µν<br />

γ )<br />

βδ


Summary<br />

◦ Starting from Dirac equation one<br />

can derive higher spin field<br />

◦ By modifying BW we examine<br />

validity of the Anti-Symmetric state


Thank You<br />

Thank You

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